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<ri:Resource created="2013-11-18T08:42:25Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>K-band spectra for 133 nearby M dwarfs</title><shortName>J/ApJ/748/93</shortName><identifier>ivo://CDS.VizieR/J/ApJ/748/93</identifier><altIdentifier>doi:10.26093/cds/vizier.17480093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rojas-Ayala B.</name></creator><creator><name>Covey K.R.</name></creator><creator><name>Muirhead P.S.</name></creator><creator><name>Lloyd J.P.</name></creator><date role="Updated">2017-07-04T07:08:36Z</date><date role="Created">2013-11-18T08:42:25Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>chemical-abundances</subject><subject>effective-temperature</subject><subject>infrared-astronomy</subject><subject>spectroscopy</subject><subject>stellar-spectral-types</subject><subject>m-stars</subject><subject>line-intensities</subject><description>We present K-band spectra for 133 nearby (d &lt; 33 pc) M dwarfs, including 18 M dwarfs with reliable metallicity estimates (as inferred from an FGK type companion), 11 M dwarf planet hosts, more than 2/3 of the M dwarfs in the northern 8 pc sample, and several M dwarfs from the LSPM catalog. From these spectra, we measure equivalent widths of the Ca and Na lines, and a spectral index quantifying the absorption due to H_2_O opacity (the H_2_O-K2 index). Using empirical spectral type standards and synthetic models, we calibrate the H_2_O-K2 index as an indicator of an M dwarf's spectral type and effective temperature. We also present a revised relationship that estimates the [Fe/H] and [M/H] metallicities of M dwarfs from their Na I, Ca I, and H_2_O-K2 measurements. Comparisons to model atmosphere provide a qualitative validation of our approach, but also reveal an overall offset between the atomic line strengths predicted by models as compared to actual observations. Our metallicity estimates also reproduce expected correlations with Galactic space motions and H{alpha} emission line strengths, and return statistically identical metallicities for M dwarfs within a common multiple system. Finally, we find systematic residuals between our H_2_O-based spectral types and those derived from optical spectral features with previously known sensitivity to stellar metallicity, such as TiO, and identify the CaH1 index as a promising optical index for diagnosing the metallicities of near-solar M dwarfs.</description><source format="bibcode">2012ApJ...748...93R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/748/93</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/V/70">V/70 : Nearby Stars, Preliminary 3rd Version (Gliese+ 1991)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/311">I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/198">III/198 : Palomar/MSU nearby star spectroscopic survey (Hawley+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/238">I/238 : Yale Trigonometric Parallaxes, Fourth Edition (van Altena+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/III/114">III/114 : Spectra of Late-Type Standards, 2.0-2.5 Microns (Kleinmann+ 1986)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/403/1949">J/MNRAS/403/1949 : UBV(RcIc)JHK photometry of HIP nearby stars (Koen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/704/975">J/ApJ/704/975 : Rotational velocities for M dwarfs (Jenkins+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/764">J/ApJ/701/764 : Light curves for five M-dwarf stars (Fernandez+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/493/645">J/A+A/493/645 : Gl 176 radial velocities (Forveille+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/121/117">J/PASP/121/117 : Fe &amp; Ti abundances of 12 M stars (Woolf+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/785">J/AJ/135/785 : SDSS-DR5 low-mass star spectroscopic sample (West+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/622/1102">J/ApJ/622/1102 : The planet-metallicity correlation. 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